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Table 1

Hierarchical two-planet non-resonant systems with 0.1 < a1 < 0.5 AU and a1/a2 < 0.1.

Star Age m 0 m 1 m 2 a 1 e 1 a 2 e 2 ϕ I max Ref.
(name) (Gyr) (M) (MJ) (MJ) (AU) (AU) (deg) (RJup) (deg)

HD 190360 7.8 0.96 .057 1.50 0.128 0.01 3.92 0.36 219. 0.54 ~40 (1)
HD 38529 3.3 1.48 1.13 17.6 0.131 0.25 3.70 0.36 269. 1.13 ~40 (2)
HD 11964 9.6 1.12 .079 0.62 0.229 0.30 3.16 0.04 307. 0.60 ~40 (3, 4)
HD 147018 6.4 0.93 2.12 6.56 0.239 0.47 1.92 0.13 251. 1.25 ~40 (5)
HD 168443 9.8 0.99 7.66 17.2 0.293 0.53 2.84 0.21 252. 1.51 ~50 (6)
HD 74156 3.7 1.24 1.88 8.03 0.294 0.64 3.40 0.43 266. 1.23 ~20 (7, 8, 9)
HD 163607 8.6 1.09 0.77 2.29 0.360 0.73 2.42 0.12 186. 1.05 ~30 (10)

Notes. All masses mi correspond to minimum values (Ii = 90°), except for HD 38529, which has Ii = 48°; ; was estimated using Eq.(41); The maximal inclination Imax was estimated using k2Δt = 100 s, () for HD 190360 and HD 38529 starting with a1 = 0.2 AU and e1 = 0.25.

Reference. (1) Vogt et al. (2005); (2) Benedict et al. (2010); (3) Butler et al. (2006); (4) Wright et al. (2009); (5) Ségransan et al. (2010); (6) Pilyavsky et al. (2011); (7) Naef et al. (2004); (8) Bean et al. (2008); (9) Meschiari et al. (2011); (10) Giguere et al. (2012).

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